
Reasonable saturation density and the binding energy, i.e., \(\rho _0\approx 0.16\,\mathrm {fm}^{-3}\)  and \(E_0(\rho _0)\approx -16\,\mathrm {MeV}\) .

Reasonable incompressibility coefficient \(K_0\)  of SNM, e.g., \(K_0\approx 230\pm 20\,\mathrm {MeV}\)  [1]}, [2]}, [3]}, [4]}, [5]}, [6]}, [7]}, [8]}, [9]}.
If necessary the higher order coefficients like the skewness \(J_0\)  could also be taken into consideration when constructing the single-nucleon potential [10]}.

Reasonable scalar nucleon effective mass in SNM at \(\rho _0\) , e.g., \(M_{\mathrm {s}}^{\ast }/M\approx 0.8\)  [11]}, [12]}.

The kinetic energy dependence of the nucleon potential constrained by the nucleon optical potential at \(\rho _0\)  from fitting nucleon-nucleus scattering data [13]}, [14]}, [15]}.

The symmetry energy as well as its slope parameter at the saturation density about \(E_{\mathrm {sym}}(\rho _0)\approx 30\pm 4\,\mathrm {MeV},L\approx 50\pm 20\,\mathrm {MeV}\)  [16]}, [17]}, [18]}, [19]}.

At small densities the nucleon experiences an attractive potential, while as the density increases the nucleon tends to experience a repulsive potential.

